Published November 1984
| Published
Journal Article
Open
High pressure physics and chemistry in giant planets and their satellites
- Creators
-
Stevenson, D. J.
Chicago
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Abstract
The deep interiors of Jupiter, Saturn, Uranus, Neptune, and their satellites are discussed. The important issues relevant to the physics of condensed matter are identified. The discussion emphasizes H₂, H-He, H₂-H₂O, H₂-CH₄, NH₃, and CH₄.5.75H₂O. Present and future theory and experiment are of great benefit t o planetary science.
Additional Information
© 1984 Centre pour la communication scientifique directe. Contribution number 4143 of the Division of Geological and Planetary Sciences.Attached Files
Published - Stevenson_1984p97.pdf
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Stevenson_1984p97.pdf
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Additional details
- Eprint ID
- 42595
- Resolver ID
- CaltechAUTHORS:20131120-113714678
- Created
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2013-11-24Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 4143